IGCSE Physics – Motion, Forces & Energy: Rapid Review
Physical Quantities & Measurement
Base SI units: m, kg, s, A, K, mol, cd
Prefixes: k (10^3), c (10^-2), m (10^-3), μ (10^-6), n (10^-9)
Measurement tools: ruler/mm, tape, trundle wheel (length); measuring cylinder, displacement (volume); stopwatch/stop-clock (time)
Multiple readings & averaging reduce random error; reaction time affects short intervals
Scalars & Vectors
Scalar: magnitude only (distance, speed, mass, energy, time)
Vector: magnitude + direction (displacement, velocity, acceleration, force, momentum, weight)
Vector addition: head-to-tail; right-angle components via Pythagoras and \text{soh-cah-toa}
Motion
Speed: v = \frac{d}{t} (scalar)
Velocity: v = \frac{s}{t} (vector, uses displacement)
Acceleration: a = \frac{\Delta v}{\Delta t} = \frac{v-u}{t}
Free-fall (no air): g \approx 9.8\,\text{m/s^2}
Distance–time graph: gradient = speed; horizontal = rest; curve slope changing = acceleration
Speed–time graph: gradient = acceleration, area = distance; flat = constant speed
Mass, Weight & Density
Mass: amount of matter, scalar, kg
Weight: gravitational force W = mg, vector, N
Density: \rho = \frac{m}{V}; units \text{kg/m^3}
Floating: object floats if \rho{object} < \rho{fluid}; upthrust equals weight at floatation
Forces & Newton’s Laws
Resultant force = vector sum; balanced \Rightarrow zero acceleration
1st Law: constant velocity if \Sigma F = 0
2nd Law: F = ma (same direction as a)
Friction/drag oppose motion, convert mechanical to thermal energy
Circular motion: force at 90^\circ to velocity changes direction only; greater m, v or smaller r need larger force
Hooke’s Law & Springs
F = kx (extension x proportional to force until limit of proportionality)
Spring constant k in \text{N/m}; beyond elastic limit permanent deformation
Moments & Equilibrium
Moment: M = Fd_{\perp} (Nm)
Principle: for equilibrium \sum M{cw} = \sum M{acw} and \Sigma F = 0
Centre of gravity: point where weight acts; found by suspension/plumb-line
Momentum & Impulse (Extended)
Momentum: p = mv (kg m/s)
Conservation: closed system \sum p{before} = \sum p{after}
Impulse: F\Delta t = \Delta p = m(v-u)
Energy Stores & Transfers
Main stores: kinetic, gravitational, elastic, thermal, chemical, nuclear, internal, electrostatic, magnetic
Transfer pathways: mechanical (forces), electrical (charge), heating, radiation (light/sound)
Conservation: energy cannot be created/destroyed; total remains constant
Key Energy Equations
Kinetic: E_k = \frac{1}{2}mv^2
Gravitational potential: \Delta E_p = mg\Delta h
Work done: W = Fd_{\parallel} (J = N m)
Power: P = \frac{W}{t} = \frac{\Delta E}{t} (W)
Efficiency: \text{eff} = \frac{\text{useful }E\;\text{or }P}{\text{total }E\;\text{or }P} (×100 % for %)
Energy Resources (overview)
Solar (cells/panels): renewable, no fuel/CO₂; weather dependent, high initial cost
Wind/wave/tidal/hydro: renewable; site-specific, variable, habitat impact
Geothermal: reliable where volcanic; limited sites, high cost
Biofuel: renewable, carbon-neutral in theory; land use, lower energy density
Fossil fuels: high output, on-demand; non-renewable, CO₂, SO₂
Nuclear fission: huge output, low CO₂; radioactive waste, high cost, decommissioning
Nuclear fusion (research): potentially limitless clean energy; requires extremely high T & P
Pressure
Pressure on surface: p = \frac{F}{A} (Pa)
Fluid pressure change: \Delta p = \rho g \Delta h
In fluids pressure acts equally in all directions; increases with depth and density
Use these bullet points for rapid exam recall of formulas, definitions, and core principles across Motion, Forces & Energy.